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Table 3.

LDB loci in terms of Lbol, Teff and the ages derived using several evolutionary models.

Stellar LDB ages based on Lbol
association Lbol LDB Teff LDB D&M Burrows Siess Burke BT-Settl Pisa
10−3 [L] [K] [Ma] [Ma] [Ma] [Ma] [Ma] [Ma]
Alpha Persei 2857 > 70
(3222) (3113) (< 3230) (3109) (2983) (3001)
NGC 1960 3123 19.8+4.0
(3461) (3462) (3546) (3368) (3370) (3344)
IC 4665 3110 19.7+1.2
(3461) (3462) (3546) (3369) (3370) (3345)
NGC 2547 3004
(3377) (3329) (3440) (3236) (3267) (3229)
IC 2602 2926
(3342) (3265) (3351) (3191) (3203) (3160)
IC 2391 2956
(3307) (3240) (3308) (3162) (3170) (3134)
The Pleiades 2728 > 70
(3057) (2922) (< 3230) (2959) (2793) (2834)
Blanco 1 2746 > 70
(3031) (2891) (< 3230) (2935) (2758) (2800)
The Hyades 2021 > 500 > 210 > 70 > 188 > 317
(< 2265) (< 2741) (< 3230) (< 2818) (1969) (< 2331)
BPMG 3095 < 18.5 < 18.1
(3559) (> 3482) (3641) (> 3467) (3432) (3440)
THMG 2935
(3350) (3273) (3363) (3200) (3212) (3168)
32 Ori MG 3135 < 18.5 18.1+0.5
(3553) (> 3482) (3631) (3467) (3426) (3431)

32 Ori MG-P1 3157 < 18.5 18.1+4.0
(3555) (> 3482) (3634) (3467) (3427) (3433)
32 Ori MG-P2 3098 < 18.5
(3501) (> 3482) (3582) (3409) (3396) (3380)
Theia 133 3139 < 18.5+2.2 18.5+6.7
(3549) (> 3482) (3624) (3460) (3421) (3423)
Theia 370 3087 < 18.5+2.9
(3499) (> 3482) (3580) (3407) (3396) (3378)

Notes. Lbol LDB and Teff LDB are the locations of the LDB in terms of bolometric luminosity and effective temperature. The rest of the columns are the ages estimated using Lbol LDB and the next evolutionary models: D’Antona & Mazzitelli (1997; ‘D&M’), Burrows et al. (1993, 1997; ‘Burrows’), Siess et al. (2000; ‘Siess’), Burke et al. (2004; ‘Burke’), Allard et al. (2012; ‘BT-Settl’), and Tognelli et al. (2015; ‘Pisa’). We add in parenthesis, below each estimated age, the Teff LDB at which the LDB would be expected to be found, see Sect. 6.4. We added the LDB ages of the 32 Ori MG subsamples and sub-populations for completeness (see Appendix D).

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